English
Related papers

Related papers: Neutrino nonstandard interactions in the supernova

200 papers

Neutrino non-standard interactions (NSI), previously introduced for the sun, are studied in the supernova context. For normal hierarchy the probability for electron neutrinos and antineutrinos at low energy ($E\lesssim 0.8-0.9 MeV$) is…

High Energy Physics - Phenomenology · Physics 2013-04-10 C. R. Das , Joao Pulido

We consider the effect of non-standard neutrino interactions (NSI, for short) on the propagation of neutrinos through the supernova (SN) envelope within a three-neutrino framework and taking into account the presence of a neutrino…

High Energy Physics - Phenomenology · Physics 2010-04-06 A. Esteban-Pretel , R. Tomas , J. W. F. Valle

Non-standard neutrino interactions (NSI) affect both their propagation through matter and their detection, with bounds on NSI parameters coming from various astrophysical and terrestrial neutrino experiments. In this paper, we show that NSI…

High Energy Physics - Phenomenology · Physics 2017-08-31 Bhaskar Dutta , Shu Liao , Louis E. Strigari , Joel W. Walker

We investigate the prospects for non-standard interactions (NSI) in solar neutrino propagation and detection and find that these may solve the tension between the observed flatness of the SuperKamiokande electron spectrum and its LMA…

High Energy Physics - Phenomenology · Physics 2011-08-17 Joao Pulido , C. R. Das

Nonstandard interactions (NSI) of neutrinos with matter can significantly alter neutrino flavor evolution in supernovae with the potential to impact explosion dynamics, nucleosynthesis, and the neutrinos signal. In this paper, we explore,…

High Energy Physics - Phenomenology · Physics 2016-12-07 Charles J. Stapleford , Daavid J. Väänänen , James P. Kneller , Gail C. McLaughlin , Brandon T. Shapiro

We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through the detection of neutrinos produced in a future galactic supernova (SN).We consider the effect of NSI on the neutrino propagation through the…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. Esteban-Pretel , R. Tomàs , J. W. F. Valle

We consider the decoupling of neutrinos in the early Universe in presence of non-standard neutral current neutrino-electron interactions (NSI). We first discuss a semi-analytical approach to solve the relevant kinetic equations and then…

High Energy Physics - Phenomenology · Physics 2009-11-11 Gianpiero Mangano , Gennaro Miele , Sergio Pastor , Teguayco Pinto , Ofelia Pisanti , Pasquale D. Serpico

Non-standard interactions (NSI) of neutrinos with matter mediated by a scalar field would induce medium-dependent neutrino masses which can modify oscillation probabilities. Generating observable effects requires an ultra-light scalar…

High Energy Physics - Phenomenology · Physics 2020-06-03 K. S. Babu , Garv Chauhan , P. S. Bhupal Dev

Non-standard neutrino self interactions (NSSI) could be stronger than Fermi interactions. We investigate the ability to constrain these four-neutrino interactions by their effect on the flux of neutrinos originating from a galactic…

High Energy Physics - Phenomenology · Physics 2020-02-19 Minjie Lei , Noah Steinberg , James D. Wells

We show that non-standard neutrino interactions (NSI) can notably modify the pattern of resonant flavor conversion of neutrinos within supernovae and significantly impact the neutronization burst signal in forthcoming experiments such as…

High Energy Physics - Phenomenology · Physics 2025-03-25 Sudip Jana , Yago Porto

Non-standard interactions (NSI) between neutrinos and electrons can significantly modify the decoupling of neutrinos from the plasma. These interactions have two effects on the overall picture: (i) they alter neutrino oscillations though…

High Energy Physics - Phenomenology · Physics 2022-03-02 Pablo Martínez-Miravé

We analyze the prospects for studying scalar non-standard interactions (SNSI) using the neutrino burst from a Galactic supernova. SNSI modify the resonant flavor conversion and, correspondingly, the neutronization burst signal, and may be…

High Energy Physics - Phenomenology · Physics 2025-08-25 Bhaskar Dutta , Aparajitha Karthikeyan , Nityasa Mishra , Yago Porto , Louis E. Strigari

Neutrino non-standard interactions (NSI) with electrons, predicted in many extended theoretical models of particle physics, are known to alter the picture of neutrino decoupling from the cosmic plasma. We update previous analyses of…

High Energy Physics - Phenomenology · Physics 2026-03-02 Stefano Gariazzo , Jaume Moncho , Sergio Pastor , Ofelia Pisanti

Core-collapse supernova (CCSN) provides a unique astrophysical site for studying neutrino-matter interactions. Prior to the shock-breakout neutrino burst during the collapse of the iron core, a preshock $\nu_e$ burst arises from the…

High Energy Astrophysical Phenomena · Physics 2022-05-25 Xu-Run Huang , Shuai Zha , Lie-Wen Chen

We introduce a model for Non-Standard neutral current Interaction (NSI) between neutrinos and the matter fields, with an arbitrary coupling to the up and down quarks. The model is based on a new $U(1)$ gauge symmetry with a light gauge…

High Energy Physics - Phenomenology · Physics 2023-02-22 Nicolás Bernal , Yasaman Farzan

Non-Standard Interactions (NSI) between neutrinos and matter affect the neutrino flavor oscillations. Due to the high matter density in the core of the Sun, solar neutrinos are suited to probe these interactions. Using the $277$ kton-yr…

High Energy Physics - Experiment · Physics 2022-03-23 Kamiokande Collaboration , P. Weatherly , K. Abe , C. Bronner , Y. Hayato , K. Hiraide , M. Ikeda , K. Iyogi , J. Kameda , Y. Kanemura , Y. Kataoka , Y. Kato , Y. Kishimoto , S. Miki , M. Miura , S. Moriyama , T. Mochizuki , M. Nakahata , Y. Nakano , S. Nakayama , T. Okada , K. Okamoto , A. Orii , G. Pronost , K. Sato , H. Sekiya , M. Shiozawa , Y. Sonoda , Y. Suzuki , A. Takeda , Y. Takemoto , A. Takenaka , H. Tanaka , S. Tasaka , X. Wang , S. Watanabe , T. Yano , S. Han , T. Kajita , K. Kaneyuki , K. Okumura , T. Tashiro , R. Wang , J. Xia , G. D. Megias , L. Labarga , B. Zaldivar , B. W. Pointon , F. d. M. Blaszczyk , C. Kachulis , E. Kearns , J. L. Raaf , J. L. Stone , L. R. Sulak , S. Sussman , L. Wan , T. Wester , S. Berkman , S. Tobayama , J. Bian , M. Elnimr , N. J. Griskevich , W. R. Kropp , S. Locke , S. Mine , M. B. Smy , H. W. Sobel , V. Takhistov , A. Yankelevich , K. S. Ganezer , J. Hill , J. Y. Kim , I. T. Lim , R. G. Park , B. Bodur , Z. Li , K. Scholberg , C. W. Walter , L. Bernard , A. Coffani , O. Drapier , A. Giampaolo , S. El Hedri , J. Imber , Th. A. Mueller , P. Paganini , B. Quilain , A. D. Santos , T. Ishizuka , T. Nakamura , J. S. Jang , J. G. Learned , S. Matsuno , S. Cao , J. Amey , L. H. V. Anthony , R. P. Litchfield , W. Y. Ma , D. Martin , M. Scott , A. A. Sztuc , Y. Uchida , M. O. Wascko , V. Berardi , M. G. Catanesi , R. A. Intonti , E. Radicioni , N. F. Calabria , L. N. Machado , G. De Rosa , G. Collazuol , F. Iacob , M. Lamoureux , M. Mattiazzi , N. Ospina , L. Ludovici , M. Gonin , Y. Maekawa , Y. Nishimura , M. Friend , T. Hasegawa , T. Ishida , M. Jakkapu , T. Kobayashi , T. Matsubara , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , T. Boschi , F. Di Lodovico , J. Gao , T. Katori , J. Migenda , M. Taani , S. Zsoldos , KE. Abe , M. Hasegawa , Y. Isobe , Y. Kotsar , H. Miyabe , H. Ozaki , T. Sugimoto , A. T. Suzuki , Y. Takeuchi , S. Yamamoto , Y. Ashida , J. Feng , T. Hayashino , S. Hirota , M. Jiang , T. Kikawa , M. Mori , T. Nakaya , R. A. Wendell , K. Yasutome , P. Fernandez , N. McCauley , P. Mehta , A. Pritchard , K. M. Tsui , Y. Fukuda , Y. Itow , H. Menjo , M. Murase , K. Frankiewicz , J. Lagoda , S. M. Lakshmi , M. Mandal , P. Mijakowski , Y. S. Prabhu , J. Zalipska , M. Jia , J. Jiang , C. K. Jung , X. Li , J. L. Palomino , G. Santucci , C. Vilela , M. J. Wilking , C. Yanagisawa , D. Fukuda , K. Hagiwara , M. Harada , H. Ishino , S. Ito , H. Kitagawa , Y. Koshio , W. Ma , S. Sakai , M. Sakuda , Y. Takahira , C. Xu , Y. Kuno , G. Barr , D. Barrow , L. Cook , A. Goldsack , S. Samani , C. Simpson , D. Wark , S. Molina Sedgwick , R. Tacik , F. Nova , J. Y. Yang , S. J. Jenkins , M. Malek , J. M. McElwee , O. Stone , M. D. Thiesse , L. F. Thompson , H. Okazawa , Y. Choi , S. B. Kim , J. W. Seo , I. Yu , A. Ichikawa , K. D. Nakamura , K. Nishijima , M. Koshiba , K. Iwamoto , K. Nakagiri , Y. Nakajima , Y. Suda , N. Taniuchi , M. Yokoyama , K. Martens , M. Murdoch , M. R. Vagins , D. Hamabe , S. Izumiyama , M. Kuze , Y. Okajima , T. Yoshida , M. Inomoto , M. Ishitsuka , H. Ito , T. Kinoshita , R. Matsumoto , M. Shinoki , T. Suganuma , M. Yonenaga , J. F. Martin , C. M. Nantais , H. A. Tanaka , T. Towstego , R. Akutsu , P. de Perio , V. Gousy-Leblanc , M. Hartz , A. Konaka , P. de Perio , N. W. Prouse , S. Chen , B. D. Xu , B. Zhang , M. Posiadala-Zezula , D. Hadley , M. Nicholson , M. O'Flaherty , B. Richards , A. Ali , B. Jamieson , P. Giorgio , Ll. Marti , A. Minamino , G. Pintaudi , S. Sano , R. Sasaki , K. Wada

The present thesis aims to be an analysis of various aspects of neutrino phenomenology in two different scenarios. On the one hand, we address the study of non-standard neutrino interactions (NSI) in accelerator and reactor terrestrial…

High Energy Physics - Phenomenology · Physics 2009-12-11 Andreu Esteban-Pretel

The possible non-standard interactions (NSIs) of neutrinos with matter plays important role in the global determination of neutrino properties. In our study we select various data sets from LHC measurements at 13 TeV with integrated…

High Energy Physics - Phenomenology · Physics 2021-02-24 DianYu Liu , ChuanLe Sun , Jun Gao

Future dark matter (DM) direct detection searches will be subject to irreducible neutrino backgrounds that will challenge the identification of an actual WIMP signal in experiments without directionality sensitivity. We study the impact of…

High Energy Physics - Phenomenology · Physics 2017-12-29 D. Aristizabal Sierra , N. Rojas , M. H. G. Tytgat

We study the effects of non-standard interactions on the oscillation pattern of atmospheric neutrinos. We use neutrino oscillograms as our main tool to infer the role of non-standard interactions (NSI) parameters at the probability level in…

High Energy Physics - Phenomenology · Physics 2016-06-21 Animesh Chatterjee , Poonam Mehta , Debajyoti Choudhury , Raj Gandhi
‹ Prev 1 2 3 10 Next ›